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<ri:Resource created="2017-10-23T08:49:10Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Galaxies &gt;~6 from the Hubble Frontier Fields</title><shortName>J/ApJ/835/113</shortName><identifier>ivo://CDS.VizieR/J/ApJ/835/113</identifier><altIdentifier>doi:10.26093/cds/vizier.18350113</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Livermore R.C.</name></creator><creator><name>Finkelstein S.L.</name></creator><creator><name>Lotz J.M.</name></creator><date role="Updated">2019-06-05T13:45:54Z</date><date role="Created">2017-10-23T08:49:10Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>photometry</subject><subject>redshifted</subject><description>We report a new analysis of the Hubble Frontier Fields clusters Abell2744 and MACS 0416 using wavelet decomposition to remove the cluster light, enabling the detection of highly magnified (&gt;50x) galaxies a factor of 10x fainter in luminosity than previous studies. We find 167 galaxies at z&gt;~6, and with this sample we are able to characterize the UV luminosity function to M_UV_=-12.5 at z~6, -14 at z~7, and -15 at z~8. We find a steep faint-end slope ({alpha}&lt; -2), and with our improved statistics at the faint end we reduce the fractional uncertainty on {alpha} to &lt;2% at z~6-7 and 4% at z~8. We also investigate the systematic uncertainty due to the lens modeling by using every available lens model individually and comparing the results; this systematic fractional uncertainty on {alpha} is &lt;4% at all redshifts. We now directly observe galaxies in the luminosity regime where some simulations predict a change in the faint-end slope of the luminosity function, yet our results provide statistically very strong evidence against any turnover in the luminosity range probed, more consistent with simulations in which stars form in lower-mass halos. Thus, we find strong support for the extension of the steep luminosity function to M_UV_=-13 at z&gt;6, consistent with the number of faint galaxies needed to reionize the universe under standard assumptions.</description><source format="bibcode">2017ApJ...835..113L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/835/113</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/164">J/ApJ/756/164 : UV galaxies in CANDELS from z=8 to z=4 (Finkelstein+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/762/L30">J/ApJ/762/L30 : CLASH: MCS J0416.1-2403 strong lensing analysis (Zitrin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/793/115">J/ApJ/793/115 : UV-continuum slopes beta for z~4-8 galaxies (Bouwens+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/443/1549">J/MNRAS/443/1549 : MACSJ0416.1-2403 strong-lensing analysis (Jauzac+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/268">J/MNRAS/444/268 : HST Frontier Fields clusters (Richard+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/800/18">J/ApJ/800/18 : HST/WFC3 observations of z~7-8 galaxies in A2744 (Atek+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/803/34">J/ApJ/803/34 : z~4-10 galaxies from HST legacy fields (Bouwens+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/71">J/ApJ/810/71 : UV mag of candidate galaxies at 3~&lt;z~&lt;8.5 (Finkelstein+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/1437">J/MNRAS/452/1437 : Abell 2744 strong-lensing analysis (Jauzac+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/811/29">J/ApJ/811/29 : GLASS. 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